2015: LADDT (Luminosity, Accretion Disk, and Dust Team)

This team, which started in Jan 2015, is combining UV, optical, and near infrared data for active galactic nuclei to look for a relation between the color of their accretion disks, the emission from their dust and their luminosity.

2013: C-CWEL (Continuing Cool WISE ExpLoration of BRC 38)

This team, which started in Jan 2013, is continuing explorations of the BRC 38 cloud that the C-WAYS team began in 2012. Much of the background information found below for the IC 2118, Lynds, CG4, and C-WAYS (of course) teams also applies to this team as well.

2013: CM4Seyferts

This team, which started in Jan 2013, is working with WISE and GALEX data to seek correlations between the infrared and ultraviolet in Seyfert galaxies. They will be looking for a diagram akin to the Hertzsprung-Russel (HR) diagram for stars.

2012: C-WAYS (Cool, Wise, And Young Stars)

This team, which started in Jan 2012, is working with Lynds 1548 and WISE data to find new young stars. Much of the background information found below for the IC 2118, Lynds, and CG4 teams also applies to this team as well.

2012: HR4AGN

This team, which started in Jan 2012, is working with WISE and GALEX data to seek correlations between the infrared and ultraviolet in active galactic nuclei (AGN). They will be looking for a diagram akin to the Hertzsprung-Russel (HR) diagram for stars.